Coronal X-ray enhancements associated with H? filament disappearances
Authors:
- 1 May 1976
- journal article
- Published by Springer Nature in Solar Physics
- Vol. 48 (1) , 159-186
Abstract
No abstract availableKeywords
This publication has 31 references indexed in Scilit:
- Structure and spectrum of quiescent prominences - Energy balance and hydrogen spectrumThe Astrophysical Journal, 1976
- Extreme-ultraviolet transients observed at the solar poleThe Astrophysical Journal, 1976
- Morphological evolution of X-ray flare structures from the rise through the decay phaseThe Astrophysical Journal, 1975
- The location of the site of energy release in a solar X-ray subflareThe Astrophysical Journal, 1975
- The Outer Solar Corona as Observed from Skylab: Preliminary ResultsThe Astrophysical Journal, 1974
- X-Ray Observations of Characteristic Structures and Time Variations from the Solar Corona: Preliminary Results from SKYLABThe Astrophysical Journal, 1973
- Extreme-Ultraviolet Emission from Solar ProminencesThe Astrophysical Journal, 1972
- Radiation from a High-Temperature Low-Density Plasma: the X-Ray Spectrum of the Solar CoronaThe Astrophysical Journal, 1971
- Magnetic Fields in Quiescent Solar Prominences. I. ObservationsThe Astrophysical Journal, 1967
- Regular Structures in the Green Solar CoronaPublications of the Astronomical Society of the Pacific, 1963